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The top documents tagged [balmer lines]

13 March 201313rd MAXI Symposium Be Be. Talk Outline 1.Introduction to Be stars 2.Decretion vs. accretion 3.Interactions in binaries 4.Concluding remarks
13 March 201313rd MAXI Symposium Be Be. Talk Outline 1.Introduction to Be stars 2.Decretion vs. accretion 3.Interactions in binaries 4.Concluding remarks
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Consequencies of the new intensity formula in many optical spectroscopy fields
Consequencies of the new intensity formula in many optical spectroscopy fields
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Lecture I: Introduction to White Dwarfs S. R. Kulkarni, E. Ofek srk/ay125
Lecture I: Introduction to White Dwarfs S. R. Kulkarni, E. Ofek srk/ay125
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The Size, Structure & Ionization of the Broad-Line Region in NGC 3227 and NGC 4051 Nick Devereux (ERAU) Emily Heaton (ERAU) May 22 nd, 2013 Naples, Italy
The Size, Structure & Ionization of the Broad-Line Region in NGC 3227 and NGC 4051 Nick Devereux (ERAU) Emily Heaton (ERAU) May 22 nd, 2013 Naples, Italy
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Understanding Atoms Chapter 42. The Bohr Model – good but not perfect! For Hydrogen and “Hydrogenic” atoms predicts the Rydberg formula For Hydrogen
Understanding Atoms Chapter 42. The Bohr Model – good but not perfect! For Hydrogen and “Hydrogenic” atoms predicts the Rydberg formula For Hydrogen
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Chapter 13 Cont’d – Pressure Effects More curves of growth How does the COG depend on excitation potential, ionization potential, atmospheric parameters
Chapter 13 Cont’d – Pressure Effects More curves of growth How does the COG depend on excitation potential, ionization potential, atmospheric parameters
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First Spectroscopic Evidence for High Ionization State and Low Oxygen Abundance in Lyα Emitters ( arXiv:1208.3260, ApJ submitted ) subaru UM @NAOJ on 16/Jan/2013
First Spectroscopic Evidence for High Ionization State and Low Oxygen Abundance in Lyα Emitters ( arXiv:1208.3260, ApJ submitted ) subaru UM @NAOJ on 16/Jan/2013
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1 Black Hole Masses from Reverberation Mapping Bradley M. Peterson The Ohio State University Collaborators: M. Bentz, S. Collin, K. Dasyra, K. Denney,
1 Black Hole Masses from Reverberation Mapping Bradley M. Peterson The Ohio State University Collaborators: M. Bentz, S. Collin, K. Dasyra, K. Denney,
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Chapter 25: Quasars and active galaxies Features of quasars Quasars and distant galaxies Seyfert and radio galaxies Active galactic nuclei Supermassive
Chapter 25: Quasars and active galaxies Features of quasars Quasars and distant galaxies Seyfert and radio galaxies Active galactic nuclei Supermassive
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Lecture 2. Examination The course is assessed in three parts: Problem sets. The problem sets and the peer reviews. One of the sets will randomly be corrected
Lecture 2. Examination The course is assessed in three parts: Problem sets. The problem sets and the peer reviews. One of the sets will randomly be corrected
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FFS at JET/Ameigs 02-09-13 FFS model Coupling Balmer positions to D10-2 thru Rydberg formula Coupling Lorentzian widths to the Griem Stark broadening formula
FFS at JET/Ameigs 02-09-13 FFS model Coupling Balmer positions to D10-2 thru Rydberg formula Coupling Lorentzian widths to the Griem Stark broadening formula
225 views
Stellar Spectra AST 112 Lecture 7. Stellar Spectra The interior of a star can be considered a “hot dense object” that emits a continuous spectrum. The
Stellar Spectra AST 112 Lecture 7. Stellar Spectra The interior of a star can be considered a “hot dense object” that emits a continuous spectrum. The
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